4.7 Article

Observation of an enhancement in e+e- → γ(1S)π+π-, γ(2S)π+π-, and γ(3S)π+π- production near √s=1.89 GeV

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PHYSICAL REVIEW D
卷 82, 期 9, 页码 -

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AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.82.091106

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资金

  1. MEXT
  2. JSPS
  3. Nagoya's TLPRC (Japan)
  4. ARC (Australia)
  5. DIISR (Australia)
  6. NSFC (China)
  7. MSMT (Czechia)
  8. DST (India)
  9. MEST (Korea)
  10. NRF (Korea)
  11. NSDC of KISTI (Korea)
  12. WCU (Korea)
  13. MNiSW (Poland)
  14. MES (Russia)
  15. RFAAE (Russia)
  16. ARRS (Slovenia)
  17. SNSF (Switzerland)
  18. NSC (Taiwan)
  19. MOE (Taiwan)
  20. DOE (USA)

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We measure the production cross sections for e(+)e(-) -> gamma(1S)pi(+)pi(-), gamma(2S)pi(+)pi(-), and gamma(3S)pi(+)pi(-) as a function of root 5 between 10.83 GeVand 11.02 GeV. The data consist of 8.1 fb(-1) collected with the Belle detector at the KEKB e(+)e(-) collider. We observe enhanced production in all three final states that does not agree well with the conventional gamma(10860) line shape. A fit using a Breit-Wigner resonance shape yields a peak mass of [10 888.4(-2.6)(+2.7)(stat) +/- 1.2(syst)] MeV/c(2) and a width of [30.7(-7.0)(+8.3)(stat) +/- 3.1(syst) MeV/c(2).

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